Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z
Paper Citation Record · LEDGER
AU or pc? Inferring the distance of magnetized plasma near FRBs from propagation diagnostics
As of 18 August 2026, this Paper Citation Record lists 13 of 13 outbound references and 0 inbound Pith citation observations for arXiv:2607.05289.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-18T06:34:40.430872+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links
A source-named dated measurement, never combined with another source.
Source: cited_works
Reference resolution
13 of 13 outbound references displayed
- verified exact2
- verified fuzzy8
- unresolved2
- parse uncertain0
- malformed identifier0
- metadata mismatch1
External citation measurements
No source-named external measurement is stored.
Outbound references
Observation 34acf6c1-71df-4482-84fa-e5c3b451a141 · outbound
This paper cites Radio Wave Propagation and the Provenance of Fast Radio Bursts.
AU or pc? Inferring the distance of magnetized plasma near FRBs from propagation diagnostics Radio Wave Propagation and the Provenance of Fast Radio Bursts
Reference 1
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-07-07T19:54:03.307518Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation c3d23cf5-4ec9-45e7-b321-c5893dfe6d21 · outbound
This paper cites an unresolved cited work.
AU or pc? Inferring the distance of magnetized plasma near FRBs from propagation diagnostics Unresolved cited work
Reference 2
- Resolution
- unresolved
- raw_fallback, observed 2026-07-07T19:54:03.411708Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation bac66761-5821-4e3f-8ae5-bbf109b32b33 · outbound
This paper cites " " " ".
AU or pc? Inferring the distance of magnetized plasma near FRBs from propagation diagnostics " " " "
Reference 3
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-07-07T19:54:03.395203Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation d4e1eef2-8e67-43c6-91e6-cabe9e5fc5e3 · outbound
This paper cites The eccentricity is set to𝑒=0.75 with an inclination angle𝑖=30 ◦ and semi-major axis𝑎=400 (unit: hrs).
AU or pc? Inferring the distance of magnetized plasma near FRBs from propagation diagnostics The eccentricity is set to𝑒=0.75 with an inclination angle𝑖=30 ◦ and semi-major axis𝑎=400 (unit: hrs)
Reference 4
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-07-07T19:54:03.402909Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation a6c01702-9125-40fd-aaa7-acd8db4b11aa · outbound
This paper cites FRB 20190520B: R.
AU or pc? Inferring the distance of magnetized plasma near FRBs from propagation diagnostics FRB 20190520B: R
Reference 5
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-07-07T19:54:03.406142Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation c89f92e8-87cc-44fb-ad5a-2f63888e0fe9 · outbound
This paper cites Pleunis et al.
AU or pc? Inferring the distance of magnetized plasma near FRBs from propagation diagnostics Pleunis et al
Reference 6
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-07-07T19:54:03.397607Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation c4090be1-0de0-45e3-b1e7-7da34df1b3f1 · outbound
This paper cites Figure 7.The variation of scattering (top) and RM (middle) of FRB 201905202B, and simultaneous depolarization fitting (bottom) in three stages.
AU or pc? Inferring the distance of magnetized plasma near FRBs from propagation diagnostics Figure 7.The variation of scattering (top) and RM (middle) of FRB 201905202B, and simultaneous depolarization fitting (bottom) in three stages
Reference 7
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-07-07T19:54:03.414401Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 6062cc39-004b-480d-b8d5-f8f1ecb03287 · outbound
This paper cites Later sim- liar scattering timescales were observed by LOFAR during the RM decrease phase (A.
AU or pc? Inferring the distance of magnetized plasma near FRBs from propagation diagnostics Later sim- liar scattering timescales were observed by LOFAR during the RM decrease phase (A
Reference 8
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-07-07T19:54:03.391970Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 5e989401-8409-4a93-a98b-228a406a379b · outbound
This paper cites The linear fitting of RM vari- ation in two stages turns out to be 0.41 rad/m2/day and -1.18 rad/m2/day, respectively.
AU or pc? Inferring the distance of magnetized plasma near FRBs from propagation diagnostics The linear fitting of RM vari- ation in two stages turns out to be 0.41 rad/m2/day and -1.18 rad/m2/day, respectively
Reference 9
- Resolution
- verified exact
- arxiv_id, observed 2026-07-07T19:54:03.334088Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 069c3862-d76b-4e5d-8a57-bb486638b40d · outbound
This paper cites Blue diamond and red hollow circles represent the FRBs observed by CHIME and FAST, respectively.
AU or pc? Inferring the distance of magnetized plasma near FRBs from propagation diagnostics Blue diamond and red hollow circles represent the FRBs observed by CHIME and FAST, respectively
Reference 10
- Resolution
- verified exact
- arxiv_id, observed 2026-07-07T19:54:03.338927Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 381779dc-50f0-44d9-9f0a-2f9756611b76 · outbound
This paper cites The DM0 contributed by the stellar wind is DMw,0 ≃𝑛 w(𝑎) ·𝑎= ¤𝑀 4𝜋𝑣 w𝜇i𝑚p𝑎2 ·𝑎 ≈5 pc cm −3𝑣 −1 w,8 ¤𝑀 10−8 𝑀⊙yr−1 𝑎 1 AU −1.
AU or pc? Inferring the distance of magnetized plasma near FRBs from propagation diagnostics The DM0 contributed by the stellar wind is DMw,0 ≃𝑛 w(𝑎) ·𝑎= ¤𝑀 4𝜋𝑣 w𝜇i𝑚p𝑎2 ·𝑎 ≈5 pc cm −3𝑣 −1 w,8 ¤𝑀 10−8 𝑀⊙yr−1 𝑎 1 AU −1
Reference 11
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-07-07T19:54:03.409251Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 3cc1db1a-930b-415c-a9a7-6e01564c4532 · outbound
This paper cites an unresolved cited work.
AU or pc? Inferring the distance of magnetized plasma near FRBs from propagation diagnostics Unresolved cited work
Reference 12
- Resolution
- unresolved
- raw_fallback, observed 2026-07-07T19:54:03.399952Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 2446b1e6-5111-4350-b54d-77fce4ae0792 · outbound
This paper cites E.3.Clumps in SNR The RM variations of FRBs could also be attributed to filaments in SNRs across the line of sight (J.
AU or pc? Inferring the distance of magnetized plasma near FRBs from propagation diagnostics E.3.Clumps in SNR The RM variations of FRBs could also be attributed to filaments in SNRs across the line of sight (J
Reference 13
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-07-07T19:54:03.389207Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Pith citing papers
No inbound Pith citation observations are available.